Results 31 to 40 of about 91,474 (277)

Magnetic-reconnection-driven Turbulence and Turbulent Reconnection Acceleration

The Astrophysical Journal, 2023
Abstract This paper employs an MHD-PIC method to perform numerical simulations of magnetic-reconnection-driven turbulence and turbulent reconnection acceleration of particles. Focusing on the dynamics of the magnetic reconnection, the properties of self-driven turbulence, and the behavior of particle acceleration, we find the following: (
Shi-Min Liang, Jian-Fu Zhang, Na-Na Gao, Hua-Ping Xiao   +3 more
openaire   +3 more sources

Theory and Applications of Non-Relativistic and Relativistic Turbulent Reconnection

, 2015
Realistic astrophysical environments are turbulent due to the extremely high Reynolds numbers. Therefore, the theories of reconnection intended for describing astrophysical reconnection should not ignore the effects of turbulence on magnetic reconnection.
A. A. Schekochihin, A. Beresnyak, A. Beresnyak, A. Bhattacharjee, A. Brandenburg, A. Chepurnov, A. Chepurnov, A. Ciaravella, A. Kupiainen, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Lazarian, A. Merloni, A.B. Rechester, Alex Lazarian, Alexei G. Kritsuk, Allen H. Boozer, Allen H. Boozer, Andrey Beresnyak, Andrey Beresnyak, B. Cerutti, B. Cerutti, B. Khiali, B.D.G. Chandran, Benjamin D. G. Chandran, Bing Zhang, C. B. Singh, C. Thompson, C. Vogt, C.H. Jaroschek, C.L. Gerrard, C.S. Ng, Colin A. Norman, D. Biskamp, D. Giannios, D. Giannios, D. Montgomery, D.L. Meier, David Radice, Dimitrios Giannios, Dmitri A. Uzdensky, E M de Gouveia Dal Pino, E. Hameiri, E. M. DE GOUVEIA DAL PINO, E. M. de Gouveia Dal Pino, E.N. Parker, E.N. Parker, E.T. Vishniac, Elisabete M. de Gouveia Dal Pino, Ellen G. Zweibel, Ethan T. Vishniac, Eun‐jin Kim, F. Heitsch, F. Heitsch, F.H. Shu, Fan Guo, G. Brunetti, G. Drenkhahn, G. Eyink, G. Kowal, G. Kowal, G. Kowal, G. Lapenta, G. Lapenta, G. Rocha da Silva, Gregory L. Eyink, Grzegorz Kowal, Grzegorz Kowal, Grzegorz Kowal, H. Alfvén, H. Karimabadi, H. Karimabadi, H. Tennekes, H.R. Strauss, I.V. Sytine, J. Cho, J. F. Drake, J.C. Higdon, J.F. Drake, J.F. Drake, J.T. Gosling, J.V. Shebalin, J.W. Armstrong, Jason Maron, Jeffrey S. Oishi, Jonathan C. McKinney, Jonathan Zrake, Jonathan Zrake, Jungyeon Cho, Jungyeon Cho, Jungyeon Cho, Jungyeon Cho, Jungyeon Cho, Jungyeon Cho, K. Kulpa-Dybeł, K. Subramanian, Katia M. Ferrière, Kazunari Shibata, Klaus Galsgaard, Kris Beckwith, L. H. S. Kadowaki, L. O’C. Drury, L.F. Burlaga, Lorenzo Sironi, M. Hoshino, M. R. M. Leão, M. Takamoto, M. Yamada, M.A. Shay, M.A. Shay, Makoto Takamoto, Marco Fatuzzo, Maxim Lyutikov, N. F. Loureiro, N. F. Loureiro, Olga Khabarova, P. Browning, P. G. Watson, P. Goldreich, P.A. Sweet, P.H. Diamond, P.S. Iroshnikov, Padeli P. Papadopoulos, Paolo Padoan, R. Narayan, R. Santos-Lima, R. Santos-Lima, R. Santos-Lima, R. Sych, R.H. Kraichnan, R.J. Leamon, Ramesh Narayan, S. GALTIER, S. Galtier, S. S. Komissarov, S. Servidio, S. Stanimirović, S. Zenitani, S. Zenitani, S.A. Balbus, S.I. Syrovatskii, Seiji Zenitani, Stanislav Boldyrev, Stanislav Boldyrev, T. A. Enßlin, Tsuyoshi Inoue, W.H. Matthaeus, W.H. Matthaeus, W.H. Matthaeus, Weiqun Zhang, Y.E. Litvinenko, Yoram Lithwick, Z.B. Guo, Z.S. She   +164 more
core   +1 more source

Eruption and Interplanetary Evolution of a Stealthy Streamer-Blowout CME Observed by PSP at ∼0.5 AU

Frontiers in Astronomy and Space Sciences, 2022
Streamer-blowout coronal mass ejections (SBO-CMEs) are the dominant CME population during solar minimum. Although they are typically slow and lack clear low-coronal signatures, they can cause geomagnetic storms.
Sanchita Pal, Benjamin J. Lynch, Simon W. Good, Erika Palmerio, Eleanna Asvestari, Jens Pomoell, Michael L. Stevens, Emilia K. J. Kilpua   +7 more
doaj   +1 more source

Astrophysical Implications of Turbulent Reconnection: from cosmic rays to star formation

, 2005
Turbulent reconnection allows fast magnetic reconnection of astrophysical magnetic fields. This entails numerous astrophysical implications and opens new ways to approach long standing problems.
Lazarian, A.
core   +2 more sources

Rate of steady-state reconnection in an incompressible plasma [PDF]

, 2001
The reconnection rate is obtained for the simplest case of 2D symmetric reconnection in an incompressible plasma. In the short note (Erkaev et al., Phys. Rev.
Helfried K. Biernat, Ilya V. Alexeev, Nikolai V. Erkaev, Pudovkin M. I., Vladimir S. Semenov   +4 more
core   +2 more sources

Fractal Reconnection in Solar and Stellar Environments

, 2016
Recent space based observations of the Sun revealed that magnetic reconnection is ubiquitous in the solar atmosphere, ranging from small scale reconnection (observed as nanoflares) to large scale one (observed as long duration flares or giant arcades ...
A. Asai, A. Bemporad, A. Bhattacharjee, A. Veronig, A.R. Inglis, B.E. Schaefer, B.T. Tsurutani, C.D. Pike, C.Z. Cheng, D. Biskamp, D. Biskamp, D. Nogami, D.A. Uzdensky, D.E. McKenzie, D.E. McKenzie, D.M. Alexander, E. Pariat, E.N. Parker, E.P. Rubenstein, E.R. Priest, F. Miyake, F. Miyake, F. Moreno-Insertis, G.S. Choe, H. Isobe, H. Isobe, H. Ji, H. Kurokawa, H. Maehara, H. Maehara, H.P. Furth, J. Qiu, J. Zhang, J.A. Miller, J.E. Leake, J.F. Drake, J.W. Cirtain, K. A. P. Singh, K. Koyama, K. Nishida, K. Nishida, K. Ohki, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K. Shibata, K.A.P. Singh, K.A.P. Singh, L. Ni, L.-J. Guo, M. Aschwanden, M. Bárta, M. Karlicky, M. Ohyama, M. Ohyama, M. Shimizu, M. Shimojo, M. Shimojo, M. Takamoto, M. Yamada, M.G. Linton, Masamitsu Ohyama, N. Nishizuka, N. Nishizuka, N. Nishizuka, N. Nishizuka, N.F. Loureiro, N.F. Loureiro, P.A. Cassak, P.A. Cassak, P.A. Sturrock, P.F. Wyper, R. Samtaney, R.A. Kopp, R.C. Carrington, R.L. Fermo, S. Masuda, S. Notsu, S. Takasao, S. Takasao, S. Tanuma, S. Tsuneta, S. Tsuneta, S. Tsuneta, S. Zenitani, S. Zenitani, T. Hirayama, T. Magara, T. Shibayama, T. Tajima, T. Terasawa, T. Yokoyama, T. Yokoyama, T. Yokoyama, T. Yokoyama, U. Feldman, V. Archontis, W. Daughton, Y. Notsu, Y. Ono, Y.-M. Huang, Y.-M. Huang, Y.-M. Huang, Yuta Notsu, Z. Mei   +110 more
core   +1 more source

On the 3-D structure and dissipation of reconnection-driven flow-bursts [PDF]

, 2014
The structure of magnetic reconnection-driven outflows and their dissipation are explored with large-scale, 3-D particle-in-cell (PIC) simulations. Outflow jets resulting from 3-D reconnection with a finite length x-line form fronts as they propagate ...
Cassak, P. A., Drake, J. F., Phan, T. D., Swisdak, M.   +3 more
core   +3 more sources

Forced Magnetic Reconnection [PDF]

Physica Scripta, 1982
By studying a simple model problem, the time evolution of magnetic field islands which are induced by perturbing the boundary surrounding an incompressible plasma with a resonant surface inside is examined. The reconnection and island formation process for sufficiently small boundary perturbations occurs on the tearing mode time scale defined by Furth,
Hahm, T. S., Kulsrud, R. M.
openaire   +2 more sources

Where should MMS look for electron diffusion regions?

, 2015
A great possible achievement for the MMS mission would be crossing electron diffusion regions (EDR). EDR are regions in proximity of reconnection sites where electrons decouple from field lines, breaking the frozen in condition.
Goldman, M., Lapenta, G., Markidis, S., Newman, D.   +3 more
core   +1 more source

Forced magnetic reconnection and plasmoid coalescence: I - MHD Simulations [PDF]

, 2019
Forced magnetic reconnection, a reconnection event triggered by external perturbation, should be ubiquitous in the solar corona. Energy released during such cases can be much greater than that which was introduced by the perturbation.
Browning, Philippa, Gordovskyy, Mykola, Potter, Max   +2 more
core   +2 more sources